Chemical ordering and composition fluctuations at the (001) surface of the Fe64Ni36 Invar alloy

M. Ondráček1, F. Máca1, J. Kudrnovský1, J. Redinger2,4, A. Biedermann3, C. Fritscher2,5, M. Schmid2, P.Varga2

1 Institute of Physics ASCR, 18221 Praha 8, Czech Republic
2 Institut für Allgemeine Physik, Technische Universität Wien, 1040 Wien, Austria
3 Institut für Materialphysik, Universität Wien, 1090 Wien, Austria
4 Center for Computational Materials Science, Technische Universität Wien, Austria
5Present address: Institut für Werkstoffwissenschaft und Werkstofftechnologie, Technische Universität Wien, Austria

Phys. Rev. B 74 (2006) 235437

We report on a study of (001) oriented fcc Fe-Ni alloy surfaces which combines first-principles calculations and low-temperature scanning tunneling microscopy (STM) experiments. Density functional theory calculations show that Fe-Ni alloy surfaces are buckled with the Fe atoms slightly shifted outwards and the Ni atoms inwards. This is consistent with the observation that the atoms in the surface layer can be chemically distinguished in the STM image: brighter spots (corrugation maxima with increased apparent height) indicate iron atoms, darker ones nickel atoms. This chemical contrast reveals a c(2x2) chemical order (50% Fe) with frequent Fe-rich defects on the Fe64Ni36(001) surface. The calculations also indicate that subsurface composition fluctuations may additionally modulate the apparent height of the surface atoms. The STM images show that this effect is pronounced compared to the surfaces of other disordered alloys, which suggests that some chemical order and corresponding concentration fluctuations exist also in the subsurface layers of Invar alloy. In addition, detailed electronic structure calculations allow us to identify the nature of a distinct peak below the Fermi level observed in the tunneling spectra. This peak corresponds to a surface resonance band which is particularly pronounced in iron-rich surface regions and provides a second type of chemical contrast with less spatial resolution but one that is essentially independent of the subsurface composition.

Corresponding author: F. Máca. Reprints also available from M. Schmid (schmid< encoded email address >).

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A preprint is available at arXiv.org.